'Radial distribution' presentation slideshows

Non-Baryonic Dark Matter in Cosmology

784 views • 59 slides

Physical Chemistry III (01403342) Chapter 3: Atomic Structure

Physical Chemistry III (01403342) Chapter 3: Atomic Structure. Piti Treesukol Kasetsart University Kamphaeng Saen Campus. Electronic Structures of Atoms. Hydrogenic atoms Many-electron atoms The orbital approximations Self-consistent Field orbitals Approximation Methods Variation Method

761 views • 48 slides

Observational Test of Halo Model: an empirical approach

Observational Test of Halo Model: an empirical approach. Mehri Torki. Bob Nichol. The Halo-model of clustering. (lahmu.phyast.pitt.edu/~sheth/courses/allahabad/halomodel.ppt). Two types of pairs: both particles in same halo, or particles in different halos ? dm (r) = ? 1h (r) + ? 2h (r)

607 views • 45 slides

Physical Chemistry 2 nd Edition

707 views • 38 slides

Spatial distribution of luminous X-ray binaries in galaxies

Spatial distribution of luminous X-ray binaries in galaxies. introduction. Chandra observations have revolutionized XRB studies with the discovery of large numbers of point X-ray sources in galaxies even beyond the Local Group (Fabbiano et al. 2003)

391 views • 27 slides

Stellar populations in

- Ringberg Castle, July 15, 200 8 -. First results from LBC imaging:. Stellar populations in. Galactic Globular Clusters. Giacomo Beccari Astronomy Dept. - Bologna University (ITALY).

339 views • 22 slides

Transmission System Reactive Compensation and Stability Enhancement Using 48-pulse Static Synchronous Series Compensator

Transmission System Reactive Compensation and Stability Enhancement Using 48-pulse Static Synchronous Series Compensator (SSSC). A.M. Sharaf & M. S. El-Moursi Department of Electrical/Computer Engineering, University of New Brunswick PO Box 4400-UNB, Fredericton, N.B., Canada, E3B 5A3

693 views • 20 slides

Transmission System Reactive Compensation and Stability Enhancement Using 48-pulse Static Synchronous Series Compensator

Transmission System Reactive Compensation and Stability Enhancement Using 48-pulse Static Synchronous Series Compensator (SSSC). A.M. Sharaf & M. S. El-Moursi Department of Electrical/Computer Engineering, University of New Brunswick PO Box 4400-UNB, Fredericton, N.B., Canada, E3B 5A3

403 views • 20 slides

Transmission System Reactive Compensation and Stability Enhancement Using 48-pulse Static Synchronous Series Compensator

Transmission System Reactive Compensation and Stability Enhancement Using 48-pulse Static Synchronous Series Compensator (SSSC). A.M. Sharaf & M. S. El-Moursi Department of Electrical/Computer Engineering, University of New Brunswick PO Box 4400-UNB, Fredericton, N.B., Canada, E3B 5A3

583 views • 20 slides

Star Formation History of M100: Swift/UVOT

Star Formation History of M100: Swift/UVOT. Alison Newell, Ignacio Ferreras & Mark Cropper Mullard Space Science Laboratory, University College London. Scope of talk. Describe current UV Imaging Surveys M100 (NGC 4321) Describe the data Models of Unresolved Stellar Populations

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Atomistic Visualization: On-the-fly Data Extraction and Rendering

Atomistic Visualization: On-the-fly Data Extraction and Rendering. Dipesh Bhattarai Dr. Bijaya B. Karki Department of Computer Science Louisiana State University. ACMSE 2007: The 45 th ACM Southeast Conference Winston-Salem, North Carolina, USA March 23-24, 2007. Presentation Outline.

328 views • 20 slides

280 views • 16 slides

Radio Sources in High-Redshift Galaxy Clusters: An Initial Look

Radio Sources in High-Redshift Galaxy Clusters: An Initial Look. Megan Roscioli University of Chicago In collaboration with Mike Gladders, U. Chicago RCS-1,2 Collaboration. GLCW8, Columbus. Motivation.

234 views • 15 slides

Inverse Abel transform

Inverse Abel transform. Kaarel Piip 2 nd year PhD student Institute of Physics. Outline. Idea of the Abel transform Analytical formula for the inverse transform Application to experimental problems Data processing and numerical algorithms Con c lusions. Abel transform.

1.58k views • 11 slides

Radial Distribution of Pions and Muons H.G. Kirk and H.K. Sayed BNL Target Studies Meeting

Radial Distribution of Pions and Muons H.G. Kirk and H.K. Sayed BNL Target Studies Meeting. August 21, 2012. The Parameter Set. H. Sayed. Taper 20T ?1.5T 15m Front End Particle Throughput 100MeV/c < P tot < 300Me/V/c Transvers Acceptance 30mm Longitudinal Acceptance 150mm.

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A NEW VPM ALGORITHM FOR REPETITIVE DIVES

A NEW VPM ALGORITHM FOR REPETITIVE DIVES. David E. Yount * University of Hawaii Honolulu, Hawaii. Eric B. Maiken n&k Technology, Inc. Santa Clara, California. Erik C. Baker Affiliated Engineers SE, Inc. Gainesville, Florida.

290 views • 1 slides

A NEW VPM ALGORITHM FOR REPETITIVE DIVES

A NEW VPM ALGORITHM FOR REPETITIVE DIVES. David E. Yount * University of Hawaii Honolulu, Hawaii. Eric B. Maiken n&k Technology, Inc. Santa Clara, California. Erik C. Baker Affiliated Engineers SE, Inc. Gainesville, Florida.

127 views • 1 slides

FR Ferraro et al. Nature 492 , 393 - 395 (2012) doi:10.1038/nature11686

The radial distribution of BSSs in systems of intermediate dynamical ages (family II). FR Ferraro et al. Nature 492 , 393 - 395 (2012) doi:10.1038/nature11686.

85 views • 1 slides

FR Ferraro et al. Nature 492 , 393 - 395 (2012) doi:10.1038/nature11686

The radial distribution of BSSs in three dynamically young stellar systems (family I). FR Ferraro et al. Nature 492 , 393 - 395 (2012) doi:10.1038/nature11686.

88 views • 1 slides